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Table A.4

Observed and fitted properties of the H2O 312–303 line for the detected intermediate- and high-mass objects.

Source rmsa b FWZI
(mK) (K) (K km s-1) (km s-1)

Inter.-mass
NGC 7129-FIRS2 14 0.46 7.48 ± 0.02 66
NGC 2071 28 2.68 58.82 ± 0.03 117
OMC-2-FIR 4 30 1.589 25.10 ± 0.11 54

High-mass
IRAS 05358+3543 30 1.20 19.29 ± 0.03 60
IRAS 16272-4837 32 0.77 11.11 ± 0.04 42
NGC 6334I-N-1 28 1.34 28.34 ± 0.03 90
W43-MM1 24 0.83 13.07 ± 0.03 85
DR21-OH 25 3.66 63.78 ± 0.03 102
W3-IRS5 81 6.78 99.98 ± 0.08 78
IRAS 18089-1732 30 1.04 15.99 ± 0.03 66
W33A 19 1.84 20.24 ± 0.02 66
IRAS 18151-1208 30 0.47 5.85 ± 0.03 40
AFGL2591 22 2.54 16.02 ± 0.03 57
G327-0.6 39 1.88 24.97 ± 0.04 57
NGC 6334-I-1 128 3.73 48.12 ± 0.12 30
G29.96-0.02 34 2.88 36.15 ± 0.04 81
G31.41+0.31 36 1.28 13.79 ± 0.04 45
G5.89-0.39 36 8.38 237.69 ± 0.04 144
G10.47+0.03 32 2.25 24.35 ± 0.04 27
G34.26+0.15 42 5.01 45.95 ± 0.05 48
W51N-e1 63 4.40 82.48 ± 0.07 110
NGC 7538-IRS1 37 3.96 27.53 ± 0.04 81

Notes. FWZI has been calculated by binning the spectra to 3 km s-1.

(a)

In 0.27 km s-1 bin.

(b)

Integrated over the interval of velocities defined by the FWZI.

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